A dark energy model in a scalar tensor theory of gravitation

Details A dark energy model in a scalar tensor theory of gravitation A dark energy model in a scalar tensor theory of gravitation

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.337..499r&link_type=abstract

Astrophysics and Space Science, Volume 337, Issue 1, pp.499-501

Mathematics

Logic

Scalar-Tensor Theory, Dark Energy Cosmological Model

Scientific paper

LRS Bianchi type-I dark energy model with variable equation of state (EoS) parameter is presented in the scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). To get a determinate solution of the field equations we take the help of special law of variation for Hubble's parameter presented by Bermann (Nuovo Cimento B 74:182, 1983) which yields a cosmological model with negative constant deceleration parameter. Some physical and kinematical properties of the model are also discussed.

Affiliated with

Also associated with

No associations

Rating

A dark energy model in a scalar tensor theory of gravitation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A dark energy model in a scalar tensor theory of gravitation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A dark energy model in a scalar tensor theory of gravitation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-750423